Formation and Collapse of False Vacuum Bubbles in Relativistic Heavy-Ion Collisions
نویسندگان
چکیده
It is possible that under certain situations, in a relativistic heavy-ion collision, partons may expand out forming a shell like structure. We analyze the process of hadronization in such a picture for the case when the quark-hadron transition is of first order, and argue that the inside region of such a shell must correspond to a supercooled (to T = 0) deconfined vacuum. Hadrons from that region escape out, leaving a bubble of pure deconfined vacuum with large vacuum energy. This bubble undergoes relativistic collapse, with highly Lorentz contracted bubble walls, and may concentrate the entire energy into extremely small regions. Eventually different portions of bubble wall collide, with the energy being released in the form of particle production. Thermalization of this system can lead to very high temperatures. With a reasonably conservative set of parameters, at LHC, the temperature of the hot spot can reach as high as 3 GeV, and well above it with more optimistic parameters. Such a hot spot can leave signals like large PT partons, dileptons, and enhanced production of heavy quarks. We also briefly discuss a speculative possibility where the electroweak symmetry may get restored in the highly dense region resulting from the decay of the bubble wall via the phenomenon of non-thermal symmetry restoration (which is usually employed in models of pre-heating after inflation). If that could happen then the possibility may arise of observing sphaleron induced baryon number violation in relativistic heavy-ion collisions. PACS numbers: 25.75.-q, 12.38.Mh, 98.80.Cq Typeset using REVTEX e-mail: [email protected] e-mail: [email protected] email: [email protected]
منابع مشابه
Modeling Magnetic Field in Heavy ion Collisions Using Two Different Nuclear Charge Density Distributions
By studying the properties of matter during heavy-ion collisions, a better understanding of the Quark-Gluon plasma is possible. One of the main areas of this study is the calculation of the magnetic field, particularly how the values of conductivity affects this field and how the field strength changes with proper time. In matching the theoretical calculations with results obtained in lab, two diffe...
متن کاملPossibility of baryon number violation at hot spots in relativistic heavy-ion collisions
It is possible that under certain situations, in a relativistic heavy-ion collision, partons may expand out forming a shell like structure. We analyze the process of hadronization in such a picture for the case when the quarkhadron transition is of first order, and argue that the inside region of such a shell must correspond to supercooled (to T = 0) deconfined vacuum. Hadrons from that region ...
متن کاملar X iv : h ep - p h / 02 04 01 4 v 1 1 A pr 2 00 2 BNL - NT - 02 / 5 Classical Chromo – Dynamics of Relativistic Heavy
Abstract. Relativistic heavy ion collisions produce thousands of particles, and it is sometimes difficult to believe that these processes allow for a theoretical description directly in terms of the underlying theory – QCD. However once the parton densities are sufficiently large, an essential simplification occurs – the dynamics becomes semi– classical. As a result, a simple ab initio approach...
متن کاملStrange Dibaryons in Neutron Stars and in Heavy-Ion Collisions
The formation of dibaryons with strangeness are discussed for the interior of neutron stars and for central relativistic heavy-ion collisions. We derive limits for the properties of H-dibaryons from pulsar data. Signals for the formation of possible bound states with hyperons at BNL’s Relativistic Heavy-Ion Collider (RHIC) are investigated by studying their weak decay patterns and production ra...
متن کاملRelativistic Hydrodynamics for Heavy–Ion Collisions I. General Aspects and Expansion into Vacuum
We present algorithms to solve relativistic hydrodynamics in 3+1–dimensional situations without apparent symmetry to simplify the solution. In simulations of heavy–ion collisions, these numerical schemes have to deal with the physical vacuum and with equations of state with a first order phase transition between hadron matter and a quark–gluon plasma. We investigate their performance for the on...
متن کامل